Explanation: In the center of the glowing red gas on the Trifid Nebula lies an open cluster of young hot stars. The energetic light from these stars strikes hydrogen atoms in the surrounding nebula causing them to lose their electrons. When an electron finds its way back to a hydrogen proton, it emits light at very specific colors - one of which is the red color of the nebula seen here. The red glow is thus indicative of an emission nebula. The dramatic dark sheets are made of interstellar dust grains, tiny needle shaped pellets which are thought to be created and expelled in the atmospheres of cooler stars.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Publikacii s klyuchevymi slovami: Trifid nebula - emissionnaya tumannost' - Trehrazdel'naya tumannost' - Mezhzvezdnaya pyl' Publikacii so slovami: Trifid nebula - emissionnaya tumannost' - Trehrazdel'naya tumannost' - Mezhzvezdnaya pyl'
Sm. takzhe: Prizraki v Kassiopee Melott 15 v tumannosti Serdce Tumannost' Tyul'pan i chernaya dyra Lebed' X-1 Svet, temnota i pyl' v Trehrazdel'noi tumannosti Triplet v Strel'ce Prekrasnaya Trehrazdel'naya tumannost' NGC 6188: drakony v Zhertvennike Vse publikacii na tu zhe temu >>